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IR STIG Seminar Monday, December 1, 2025, 3:00pm ET

We will have two presentations this month from Ben Mazin (University of California Santa Barbara) and Lindsey Wiser (Johns Hopkins Applied Physics Laboratory).  Dr. Mazin will share MKID development progress and Dr. Wiser will discuss the study of exoplanet atmospheres through transit spectroscopy. Titles and abstracts below.

Microwave Kinetic Inductance Detectors for Future NASA UVOIR Missions

Speaker

Benjamin A. Mazin (University of California Santa Barbara)

Abstract

UV, Optical, and near-IR Microwave Kinetic Inductance Detectors, or MKIDs, are superconducting detectors that can tell you the energy and arrival time of each individual photon without false counts. In this talk I will discuss the recent progress my group has made on improving MKID spectral resolution to R>30 and fielding them at some of the largest telescopes in the world. I will also discuss our efforts to ready the technology for future NASA missions like HWO.

Exoplanet Compositions, Climates, and Formation Histories from Hubble to Webb

Speaker

Lindsey Wiser (Johns Hopkins University, Applied Physics Laboratory)

Abstract

Over the past three decades, exoplanet science has progressed from the first planet detections to detailed atmospheric characterization and population-level studies. In this talk, I will explore how the James Webb Space Telescope (JWST) is transforming our understanding of transiting exoplanet atmospheres, building on a foundation laid by the Hubble and Spitzer Space Telescopes. I will briefly describe how we compare observations to atmosphere models to infer atmosphere compositions, and present examples of results pre- and post-JWST. I will highlight how these measurements inform our understanding of exoplanet climates and formation histories, including a case study of the gas giant WASP-80 b. You can find more information about IR STIG activities and past seminars here: https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/ir-stig/. As a reminder, if you or someone who works with you is not on the IRSTIG mailing list, please sign up here

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.